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D
D D
D
L A P T E V
S E A
C24 (53 Ma)
A M E R A S I A N
B A S I N
A M E R A S I A N
B A S I N
GR
EE
NL
AN
DG
RE
EN
LA
ND
ALPHA RIDGEALPHA RIDGE
D
D
D
D
L A P T E V
S E A
C24 (53 Ma)
A M E R A S I A N
B A S I N
A M E R A S I A N
B A S I N
GR
EE
NL
AN
DG
RE
EN
LA
ND
ALPHA RIDGEALPHA RIDGE
D D
D D
L A P T E V
S E A
C24 (53 Ma)
A M E R A S I A N
B A S I N
A M E R A S I A N
B A S I N
GR
EE
NL
AN
DG
RE
EN
LA
ND
ALPHA RIDGEALPHA RIDGE
1. DATA 3. CRUSTAL STRUCTURE 4. BREAK-UP SETTING
5. CENOZOIC SEDIMENTATION
1
3
4 52
-80 -60 -40 -20 0 20 40 60 80 100 120
mGal
FREE-AIR GRAVITY
1
3
4 52
Barents sea
Amunsen Basin
Nansen Basin
Gakkel Ridge
Yermak Plateau
Svalbard Franz Josef Land
Severnaya
Zemlya
m
Novaya Z
ely
a
ara
s
K
ea
N
g
G
nl
n
si
orw
eia
n-
ree
ad Ba
n
g
St. A
nna tr
ou
h
V
oni
rug
or
n t
o
h
Franz-Vic
toria
trough
Greenland
Barents sea
Amunsen Basin
Nansen Basin
Gakkel Ridge
Yermak Plateau
Svalbard Franz Josef Land
Severnaya
Zemlya
a
ma
Nov
ya Z
ely
Kara
sea
N
g
Gr
nl
nd
si
orw
eia
n-
ee
a
Ba
n
n
trough
St.
An
a
V
oni
rug
or
n t
o
h
anz
ico
rg
Fr-
Vt
ria
tou
h
Greenland
a1
a2
a3
a4 a5 a6
a10
a11
a12
a13
a14
ai2
w001
b
c
d
e
f
g
g
COT
BATHYMETRY
A series of crustal-scale geotransects illustrating the
architecture of the continental margin were constructed using
seismic reflection profiles and both inverse and forward gravity
modeling.
The applied method includes solution of the inverse gravimetric
problem with respect to the gravity effect of a thermally
differentiated mantle. An iterative grid-based gravity inversion
for Moho depth and stretching factors was applied.
Two-dimensional gravity inversion for Moho depths was
carried out along synthetic profiles taking into consideration the
distribution of sedimentary cover from sparse seismic profiles
and depth to magnetic source estimates.
The crustal transects reveal a narrow and steep continent-ocean
transition which is characteristic of sheared more than rifted
margins. This may reflect a short-lived phase of shear during
breakup prior to the opening of the Eurasia Basin which was
initiated at the Paleocene-Eocene transition.
The free-air gravity field shows large positive anomalies
associated with Plio-Pleistocene glacial fans deposited in front
of the Franz-Victoria and St. Anna troughs, which are
prominent bathymetric features in the northern Barents-Kara
Sea. These sediments were derived from uplifted and eroded
areas in the Barents-Kara Sea region.
Authors:
Alexander Minakov (Department of Earth Science, University of Bergen,
);
Jan Inge Faleide (Department of Geosciences, University of Oslo);
Vladimir Yu. Glebovsky, (VNIIOkeangeologia, Saint-Petersburg, Russia);
Rolf Mjelde (Department of Earth Science, University of Bergen)
Continental crust
Oceanic crust
Pre-Cenozoic sediments
Cenozoic sediments
-35
-30
-25
-20
-15
-10
-5
0
km
0 100 200 300 400 500 600 700 800
Franz Josef Land Western Nansen Basin
-35
-30
-25
-20
-15
-10
-5
0
km
0 100 200 300 400 500 600 700 800
Franz Josef Land Central Nansen BasinNorth Barents Basin
0 100 200 300 400 500 600 700 800
Western Nansen BasinSvalbard PlatformKong Karls Land
-35
-30
-25
-20
-15
-10
-5
0
km1
2
3
-35
-30
-25
-20
-15
-10
-5
0
km
0 100 200 300 400 500 600 700 800
Eastern Nansen BasinSt. Anna Basin St. Anna Trough
-35
-30
-25
-20
-15
-10
-5
0
km
0 100 200 300 400 500 600 700 800
North Kara Rise Voronin Trough Eastern Nansen Basin
4
5
2
Accumulation (km )
100 - 200
200 - 500
500 - 1000
> 1000
FVF
StAFVF
SF
BjF
a k R i g
G k e l d e
o eL o m n o s o v R i d g
s B iAmund en asn
o B nMakar v asi
n Ca ada
nBasi
Knip
ovi
h R
id
c
ge
Mohn Ridge
ant
nr
Si
Ana t
.
Fra
n
to
zV
icria
tr.
roni
t
Vo
n r.
Nansen Basin
ende
eev
idg
M
l
R
e
lp a R geA h id
kYerma
P tla eau
Svalbard
Gre n a de l n
Ele
mre
sean
Isld
Franz
f Jos
e
L nda
Se e n yav r a
m yaZe l
Novaya Z
em
lya
o rM r is
pJesu
iseR
Nrs
tra
it
ae
S
Lat
p
ev
SeaEurasian
Basin
Labrador Sea
w g aNor e i n
G e l dr en an
B nasi
Barents
Sea
Kar
a
a S
e
Amerasian
Basin
Bjrnaya tr.
The northern Barents Sea
continental margin has remained
the least investigated province of
the Barents Sea because of very
limited seismic data due to a
largely permanent ice cover. An
understanding of the structure
and the evolution of the
continental margin is essential to
figure out the history of
geological development and the
hydrocarbon potential of the
northern Barents Sea region.
ABSTRACT
2. METHOD
gra
in d
en
sity
-3
Density (g/cm )D
ep
th (
km
)
-1
Compaction: 0.65 km
Porosity at sea bottom: 0.52-3
Grain density: 2.7 g/cm-3
Density at sea bottom: 1.82 g/cm
ns fwe at
Deity rom
ll d a
-300 -240 -180 -120 -60 0 60 120 180 240 300 360 420
mGal
-80
-60
-40
-20
0
2004
60
80
100
30
30
60
60
90
90
80
80
58
85
BOUGUER GRAVITY
30
30
60
60
90
90
80
08
85
58
0 4 8 12 16 20 24 28 32 36 40 44 48 52 56 60 64
mln. yr.
CRUSTAL AGE
-300 -240 -180 -120 -60 0 60 120 180 240 300 360 420
mGal
0
02
04
30
30
60
60
90
09
80
80
85
85
THERMAL GRAVITY CORRECTION
-300 -240 -180 -120 -60 0 60 120 180 240 300 360 420
mGal
0-1
0
0-8
-60
4-0
-20
0
20
406080
100
120
140
30
30
60
60
90
09
80
80
85
85
MANTLE RESIDUAL ANOMALY
8 12 16 20 24 28 32 36 40
km
121416
18202224262830
23
23
32
34
34
34
30
30
60
60
09
09
80
80
58
85
1
2
34
5
MOHO DEPTH AND CRUSTAL
THICKNESS ESTIMATIONS
STRETCHING FACTORS
.1 1
1.1
1.1
1.3
1.7
52.
92. 3
.3
3.5
3.5
3.7.4 1
30
30
60
60
90
90
80
08
8558
1.0 1.5 2.0 2.5 3.0 3.5 4.0 1000
0 100 200 300 400 500 600 700 800
-35
-30
-25
-20
-15
-10
-5
0
km
0 100 200 300 400 500 600 700 800-300
-200
-100
0
100
200
300
Ma
ntle
re
sid
ua
l a
no
ma
ly
(m
Ga
l)
Distance (km)
300 Ma 58 Ma< 54 Ma
3
0 100 200 300 400 500 600 700 800-300
-200
-100
0
100
200
300
Ma
ntle
re
sid
ua
l a
no
ma
ly
(m
Ga
l)
Distance (km)
0 100 200 300 400 500 600 700 800
-35
-30
-25
-20
-15
-10
-5
0
km
300 Ma 58 Ma< 54 Ma
1
input residual
gravity anomaly
calculated anomaly
from inverted Moho
calculated anomaly
from isostatic Moho
depth to magnetic
sources estimates
Moho inverted
from gravity
Moho according to
local isostasy
Moho according to
regional isostasy
theoretical subsidence
corrected for sedimentary
load
-4 -6 -8 -10 -12 -14 -16 -18 -20
14
16
18
20
22
24
26
0.8754
3.322
14.82
0.0681
0.1595
0.3697
0.017
0.0193
0.0346
Dr=0.4
g/c
m3
Dr=0.6
g/c
m3
Dr=0.5
g/c
m3
RMS increases
Thickening of the continental crust
Oceanic Moho depth estimates (km)
Do
wn
wa
rd c
on
tin
ua
tio
n d
ep
th (
km
)
RM
S in
cre
ase
s
GRAVITY
ISOSTASY
2
2
1>Crustal density
1
2
1
SENSITIVITY TO CRUSTAL DENSITY CHANGE AND
DOWNWARD CONTINUATION DEPTH
3D GRAVITY INVERSION INCORPORATING LITHOSPHERE THERMAL GRAVITY ANOMALY
2D GRAVITY INVERSION INCORPORATING LITHOSPHERE THERMAL GRAVITY CORRECTION,
EXPONENTIAL DENSITY-DEPTH FUNCTION IN SEDIMENTS AND ISOSTATIC CONSTRAINTS
-2 00
-100
-100
-100
0-1 0
0-1 0
-100
-100 -1
00
0-1
0
-100
-100
-100
-100
1-00
10
-0
-100- 001
-100
-100
-100
-50
-50
-50
-50
-50
-50
50
-
-50
-50
-50 -50
5- 0
-50
5-0
-50
-50
-50
-50 -5
0
-50
0-5
-50
-50
- 05
-50
-50
0-5
-50
-50
5- 0
-50
0-5
-50
-50
-50
-50
-50
-50
-50
-50
-50
-50
-50
-50
-50
-25
-25
-25
-25
-25
2-5
-25
5-2
5-2
2- 5
-25
-25-25
- 52
-52
-25
-25
-25
-25
-25
2- 5
-25
-25
5-2
-25
5-2
-25
2-5
-25
-25
5-2
-25
-25
-25
-25
5-2
-25
-25
-25 -25
-25
2-5-2
5
2- 5 -25
-25
2-5
-25
-25 -25
-5
2
-25-25
-25
25-
-25
2- 5
-25
-25
-25
-25
25
-
-25
5-2
-25
-25
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0 0
00
0
00
0
0
0 0
0
0
0
0
0
0
0
00
0
0
0
00
0
0
0
0
0
0
0
0
0
00
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
0
25
25
25
25
25
25
25
25
25
25
2525
25 25
25
52
5252
25
25
25
25 25
2525
25
2525
25
2525
25
25
25
25
25
25
25
25 25
25
25
25
25
25
25
25
25
25
25
25
25
25
25
25
25
25
25
52
25
25
52
25
50
50
50
50
50
50
50
50
05
50
50
50
50
50
50
50
05
50
5050
50
05
50
05
50
50
50
5050
50
50
50
05
5050
50
100
100
100
01
0
010
100
100
010
100
1000
10
100
100
01 0
100
100
100
100
100
10001
0
100100
010
01
0
100
100
100
20020
0
200
200
200
20
0
200
200
020
200
040
400
0
0
30 6
0
60
90
120
120
-3 0
70
70
75
75
0
8
80
85
85
24n (53)
24n (53)
20n (43)
20n (43)
18n (40)
18n (40)
13n (33)
13n (33)
6n (20)
6n (20)
5n (11)
5n (11)
2an (3.5)
2an (3.5)
1
2
3
45
MAGNETIC ANOMALIES
0 200 400 600 800
nT
S N
SOME CONSTRAINTS FOR SCENARIOS OF THE NORTHERN BARENTS SEA MARGIN EVOLUTION
-The sedimentary cover in the Nansen Basin was influenced bythree large fans (Franz Victoria, Saint Anna and Voronin) whichare well pronounced in the modern sea floor topography and freeair gravity;-The sedimentary thickness in the Nansen Basin was estimated asabout 2-4 km; -It is believed that the one third of that thickness was createdduring Late Cenozoic due to Pliocene-Pleistocene uplift andglacial erosion events;-It is predicted 3-4 km stronger lithified sediments below theupper unit in front of St. Anna Trough.
- The Northern Barents/Kara continental margin is characterized by narrow continent ocean transition (50 - 80
km);
- Crustal thickness increases from the inner part of the northern Barents Sea area to the periphery constituting
20-27 km and 30 - 34 km of the crystalline crust, respectively;
- North Kara Sea area was modeled with 30 km of the crystalline crust throughout;
- The oceanic crust is thinned to around 5 km in the Nansen Basin;
- Sediment thickness decreases from 6-13 km to 1-4 km from the inner shelf towards the continent ocean
transition;
It is believed that the most probable mechanism for the formation of the
narrow northern Barents/Kara Sea margin was a short-lived episode of
shear/transtension connected to Labrador Sea/Baffin Bay spreading system
56-69 Ma
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